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Paper Citation Record · LEDGER

Extreme mass ratio inspirals around topological stars

As of 17 August 2026, this Paper Citation Record lists 82 of 82 outbound references and 3 inbound Pith citation observations for arXiv:2504.16156.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2504.16156 v2

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measured 82 of 82 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-16T11:17:28.524800Z

measured 85 of 85 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:32:36.527524Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-17T22:50:25.881325Z

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82 of 82 outbound references displayed

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Outbound references

Observation bdb77bdb-1422-4cc4-9256-7d25b26675e3 · outbound

This paper cites an unresolved cited work.

Extreme mass ratio inspirals around topological stars Unresolved cited work

Reference 1

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Observation fcbe767e-cd36-4f3f-8fb2-68414f167bee · outbound

This paper cites The Black Hole Information Problem.

Extreme mass ratio inspirals around topological stars The Black Hole Information Problem

Reference 2

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Observation fbd2e76f-15c5-4a7e-a97b-697bd8b91538 · outbound

This paper cites Testing the nature of dark compact objects: a status report.

Extreme mass ratio inspirals around topological stars Testing the nature of dark compact objects: a status report

Reference 3

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Observation 6ed700fa-86de-418d-8582-3c495a89a999 · outbound

This paper cites Black Holes Inside and Out 2024: visions for the future of black hole physics.

Extreme mass ratio inspirals around topological stars Black Holes Inside and Out 2024: visions for the future of black hole physics

Reference 4

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Observation 715143f9-ad2b-4d4d-a471-491ddbf77dda · outbound

This paper cites Towards a Non-singular Paradigm of Black Hole Physics.

Extreme mass ratio inspirals around topological stars Towards a Non-singular Paradigm of Black Hole Physics

Reference 5

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Observation 0b2594d7-ade3-423d-b1f3-7fcecedc403b · outbound

This paper cites The information paradox: A pedagogical introduction.

Extreme mass ratio inspirals around topological stars The information paradox: A pedagogical introduction

Reference 6

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Observation c8b77d48-e1f0-40c0-9978-8d3a0de1e427 · outbound

This paper cites Fuzzballs and Microstate Geometries: Black-Hole Structure in String Theory.

Extreme mass ratio inspirals around topological stars Fuzzballs and Microstate Geometries: Black-Hole Structure in String Theory

Reference 7

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Observation 5e7f0dc3-0e2e-44cf-a8a7-8dd796beab5f · outbound

This paper cites Snowmass White Paper: Micro- and Macro-Structure of Black Holes.

Extreme mass ratio inspirals around topological stars Snowmass White Paper: Micro- and Macro-Structure of Black Holes

Reference 8

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Observation 8a5e6396-b996-4c64-902f-71662d6afb51 · outbound

This paper cites Mergers and Typical Black Hole Microstates.

Extreme mass ratio inspirals around topological stars Mergers and Typical Black Hole Microstates

Reference 9

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Observation ccc6ae95-cfc8-449c-a278-34805665cd60 · outbound

This paper cites Smooth horizonless geometries deep inside the black-hole regime.

Extreme mass ratio inspirals around topological stars Smooth horizonless geometries deep inside the black-hole regime

Reference 10

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Observation 27d3d4ab-1589-478d-9ec3-d5d2748a02a0 · outbound

This paper cites Asymptotically-flat supergravity solutions deep inside the black-hole regime.

Extreme mass ratio inspirals around topological stars Asymptotically-flat supergravity solutions deep inside the black-hole regime

Reference 11

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Observation 8d1da1ae-210d-4a6c-8520-e910b553739e · outbound

This paper cites Smooth Bubbling Geometries Without Supersymmetry.

Extreme mass ratio inspirals around topological stars Smooth Bubbling Geometries Without Supersymmetry

Reference 12

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Observation 9a5eeeb7-7b7a-49ff-bae5-0bb9542ecd76 · outbound

This paper cites Schwarzschild-like Topological Solitons.

Extreme mass ratio inspirals around topological stars Schwarzschild-like Topological Solitons

Reference 13

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Observation 57025a88-19bf-4063-831f-45e00b8830a4 · outbound

This paper cites Black-hole microstate spectroscopy: ringdown, quasinormal modes, and echoes.

Extreme mass ratio inspirals around topological stars Black-hole microstate spectroscopy: ringdown, quasinormal modes, and echoes

Reference 14

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Observation a6562326-94d3-48c6-9196-06c15a7d1c35 · outbound

This paper cites Topological Stars and Black Holes.

Extreme mass ratio inspirals around topological stars Topological Stars and Black Holes

Reference 15

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Observation a88825d0-70ab-4d1c-b735-fea988460533 · outbound

This paper cites Imaging Topological Solitons: the Microstructure Behind the Shadow.

Extreme mass ratio inspirals around topological stars Imaging Topological Solitons: the Microstructure Behind the Shadow

Reference 16

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Observation 5a8c4f0b-b029-4fd0-b004-3b4c412b105c · outbound

This paper cites Cavity effect in the quasinormal mode spectrum of topological stars.

Extreme mass ratio inspirals around topological stars Cavity effect in the quasinormal mode spectrum of topological stars

Reference 17

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Observation 62a8d7d9-c3bc-4f93-b9a8-1b944731f324 · outbound

This paper cites On the stability and deformability of top stars.

Extreme mass ratio inspirals around topological stars On the stability and deformability of top stars

Reference 18

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Observation 08586111-6fb5-4546-9c3c-6e82c6696e33 · outbound

This paper cites Spectroscopy of magnetized black holes and topological stars.

Extreme mass ratio inspirals around topological stars Spectroscopy of magnetized black holes and topological stars

Reference 19

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Observation d5bcdb01-7cba-4e05-b1cb-ac096da0031f · outbound

This paper cites Non-spinning tops are stable.

Extreme mass ratio inspirals around topological stars Non-spinning tops are stable

Reference 20

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Observation 70d4f83e-557e-4304-b563-3d5b12070a34 · outbound

This paper cites Scalar perturbations in a Top-Star spacetime.

Extreme mass ratio inspirals around topological stars Scalar perturbations in a Top-Star spacetime

Reference 21

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Observation 30725a6b-6843-4233-9317-124455524bd2 · outbound

This paper cites Charge (in)stability and superradiance of Topological Stars.

Extreme mass ratio inspirals around topological stars Charge (in)stability and superradiance of Topological Stars

Reference 22

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Observation 810263de-5958-417c-bbb7-ab376c8e50e2 · outbound

This paper cites Nonradial stability of topological stars.

Extreme mass ratio inspirals around topological stars Nonradial stability of topological stars

Reference 23

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Observation 3071a68d-c17d-49b3-8b1c-bc41c4ad06f0 · outbound

This paper cites Black Strings and p-Branes are Unstable.

Extreme mass ratio inspirals around topological stars Black Strings and p-Branes are Unstable

Reference 24

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Observation 489bb06f-c3d4-41f2-8a0b-347eb8e3efa4 · outbound

This paper cites New stable phase of non-uniform charged black strings.

Extreme mass ratio inspirals around topological stars New stable phase of non-uniform charged black strings

Reference 25

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Observation ff22cddd-9e4c-4d43-a49f-6fcee5e09a15 · outbound

This paper cites Magnetic Charge Can Locally Stabilize Kaluza-Klein Bubbles.

Extreme mass ratio inspirals around topological stars Magnetic Charge Can Locally Stabilize Kaluza-Klein Bubbles

Reference 26

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Observation 43c2a049-eab7-47e7-b6af-7c44c6be61af · outbound

This paper cites Stability of topological solitons, and black string to bubble transition.

Extreme mass ratio inspirals around topological stars Stability of topological solitons, and black string to bubble transition

Reference 27

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Observation f45ea11c-2b9a-44a5-ab1a-51e90624ad06 · outbound

This paper cites Scalar waves in a Topological Star spacetime: self-force and radiative losses.

Extreme mass ratio inspirals around topological stars Scalar waves in a Topological Star spacetime: self-force and radiative losses

Reference 28

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Observation 4e7c7835-28b6-44e0-9a45-865a83d4f907 · outbound

This paper cites Scalar waves from unbound orbits in a TS spacetime: PN reconstruction of the field and radiation losses in a self-force approach.

Extreme mass ratio inspirals around topological stars Scalar waves from unbound orbits in a TS spacetime: PN reconstruction of the field and radiation losses in a self-force approach

Reference 29

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Observation 55c69185-8c6d-4735-9571-7a7a016961b9 · outbound

This paper cites LISA Definition Study Report.

Extreme mass ratio inspirals around topological stars LISA Definition Study Report

Reference 30

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Observation 05ed6701-ea3c-4a5c-a0f8-938eb94e93d4 · outbound

This paper cites Detecting Subsolar-Mass Primordial Black Holes in Extreme Mass-Ratio Inspirals with LISA and Einstein Telescope.

Extreme mass ratio inspirals around topological stars Detecting Subsolar-Mass Primordial Black Holes in Extreme Mass-Ratio Inspirals with LISA and Einstein Telescope

Reference 31

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Observation 9f23b28a-4c5a-4129-982d-a6c610d9aa48 · outbound

This paper cites The motion of point particles in curved spacetime.

Extreme mass ratio inspirals around topological stars The motion of point particles in curved spacetime

Reference 32

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Observation c6669c59-6186-4e8b-be08-d8ce67f5de0e · outbound

This paper cites Self-force and radiation reaction in general relativity.

Extreme mass ratio inspirals around topological stars Self-force and radiation reaction in general relativity

Reference 33

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Observation f7437738-e69f-4702-94b1-53396039f39e · outbound

This paper cites Gravitational-Wave Signature of an Inspiral into a Supermassive Horizonless Object.

Extreme mass ratio inspirals around topological stars Gravitational-Wave Signature of an Inspiral into a Supermassive Horizonless Object

Reference 34

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Observation 7d37be39-9c03-4ae8-b1ef-1445762bc76e · outbound

This paper cites Into the lair: gravitational-wave signatures of dark matter.

Extreme mass ratio inspirals around topological stars Into the lair: gravitational-wave signatures of dark matter

Reference 35

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Observation ea3d3f17-5ce1-469d-8807-c3e4fe89099f · outbound

This paper cites Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals.

Extreme mass ratio inspirals around topological stars Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals

Reference 36

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Observation 2579efde-84e8-41d5-af54-491a8d976994 · outbound

This paper cites Love in Extrema Ratio.

Extreme mass ratio inspirals around topological stars Love in Extrema Ratio

Reference 37

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Observation d816d439-53e5-46ce-9dce-3a628bd2a6fd · outbound

This paper cites Extreme Love in the SPA: constraining the tidal deformability of supermassive objects with extreme mass ratio inspirals and semi-analytical, frequency-domain waveforms.

Extreme mass ratio inspirals around topological stars Extreme Love in the SPA: constraining the tidal deformability of supermassive objects with extreme mass ratio inspirals and semi-analytical, frequency-domain waveforms

Reference 38

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Observation bbfe790e-0985-4d77-ad62-d103eccad561 · outbound

This paper cites Distinguishing fuzzballs from black holes through their multipolar structure.

Extreme mass ratio inspirals around topological stars Distinguishing fuzzballs from black holes through their multipolar structure

Reference 39

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source=pdf_text observed=2026-08-16T11:17:28.351415Z digest=sha256:555d4408f5857657aba7899975a27edfe1449ab5fc273d91cb4bebb79221acce

Observation 13242b9a-0bfe-4cb2-aaa9-c89ab7e99b59 · outbound

This paper cites Extreme-mass-ratio inspirals into rotating boson stars: nonintegrability, chaos, and transient resonances.

Extreme mass ratio inspirals around topological stars Extreme-mass-ratio inspirals into rotating boson stars: nonintegrability, chaos, and transient resonances

Reference 40

Resolution
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source=pdf_text observed=2026-08-16T11:17:28.355404Z digest=sha256:deb5f135e090889e04f156edc6179b0297c27e7bdf6755b87db54c3f17f9c279

Observation dad173ed-060b-45aa-9917-35e00645bff8 · outbound

This paper cites Parameterized Non-circular Deviation from the Kerr Paradigm and Its Observational Signatures: Extreme Mass Ratio Inspirals and Lense-Thirring Effect.

Extreme mass ratio inspirals around topological stars Parameterized Non-circular Deviation from the Kerr Paradigm and Its Observational Signatures: Extreme Mass Ratio Inspirals and Lense-Thirring Effect

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.359495Z

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source=pdf_text observed=2026-08-16T11:17:28.359495Z digest=sha256:d17810597b715cbe209572bd19f127a8f0477f7948fd0fe331d3675b0874325d

Observation 6ed83b6e-e0a5-4913-8e36-b650d5ac69ac · outbound

This paper cites Gravitational waves from extreme mass-ratio inspirals in Dynamical Chern-Simons gravity.

Extreme mass ratio inspirals around topological stars Gravitational waves from extreme mass-ratio inspirals in Dynamical Chern-Simons gravity

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.363528Z

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source=pdf_text observed=2026-08-16T11:17:28.363528Z digest=sha256:058b0f33b36f1cf203c0f99d96835de916ef8b887dd235a2b0cf7b9b59f87805

Observation b76585b3-b3c2-4642-9f65-289f94f8981b · outbound

This paper cites Floating and sinking: the imprint of massive scalars around rotating black holes.

Extreme mass ratio inspirals around topological stars Floating and sinking: the imprint of massive scalars around rotating black holes

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.367636Z

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source=pdf_text observed=2026-08-16T11:17:28.367636Z digest=sha256:04dd15e76d622ed597b6cba0456926be3493e44f546c728a55c1874dff9500ab

Observation 620430cb-54e8-49bf-b2b1-54dbf0ca11e3 · outbound

This paper cites Gravitational Waves from Quasicircular Extreme Mass-Ratio Inspirals as Probes of Scalar-Tensor Theories.

Extreme mass ratio inspirals around topological stars Gravitational Waves from Quasicircular Extreme Mass-Ratio Inspirals as Probes of Scalar-Tensor Theories

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.371753Z

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source=pdf_text observed=2026-08-16T11:17:28.371753Z digest=sha256:94d77e7418f0c8398957ea496596d6b3ba9b36d30384a7a717ac62da56577e0e

Observation 79739689-2bf4-498c-a9ae-f08636258039 · outbound

This paper cites Gravitational waves in massive gravity theories: waveforms, fluxes and constraints from extreme-mass-ratio mergers.

Extreme mass ratio inspirals around topological stars Gravitational waves in massive gravity theories: waveforms, fluxes and constraints from extreme-mass-ratio mergers

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.376215Z

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source=pdf_text observed=2026-08-16T11:17:28.376215Z digest=sha256:9bc52644b4698f0e8f382802119bc731c96110fb636adca74ea889a82a0694d2

Observation c4591bf0-a22a-4303-a0af-9f865bd7aebc · outbound

This paper cites Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals.

Extreme mass ratio inspirals around topological stars Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.380373Z

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source=pdf_text observed=2026-08-16T11:17:28.380373Z digest=sha256:facd32dfdf4163c1f49a84b7487747d8ae46f6e0f4d9c5ed391d066ba2e82a15

Observation d16a8df3-1c2f-4353-929d-85b1c31b803b · outbound

This paper cites Detecting massive scalar fields with Extreme Mass-Ratio Inspirals.

Extreme mass ratio inspirals around topological stars Detecting massive scalar fields with Extreme Mass-Ratio Inspirals

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.385129Z

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source=pdf_text observed=2026-08-16T11:17:28.385129Z digest=sha256:704e3dbbc860cfd1207f773c939151593f11a797af72d5d369b944dd9b814715

Observation 408cf63c-b42d-4c7b-a6fe-ce905022738c · outbound

This paper cites Speri, S.

Extreme mass ratio inspirals around topological stars Speri, S

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.389193Z

Source-reported events for the cited work

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source=pdf_text observed=2026-08-16T11:17:28.389193Z digest=sha256:add209192f6388d02f4f66ffc7e577724ac664da440004e09027e73e98f1fbde

Observation b48ea329-6feb-4b97-83d8-802b42fbd12e · outbound

This paper cites Prospects for Fundamental Physics with LISA.

Extreme mass ratio inspirals around topological stars Prospects for Fundamental Physics with LISA

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.392467Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.392467Z digest=sha256:41d329bef735d544e4eabf83d4c6cc8866f6e6a3ff4410284ce74a8816d46d9e

Observation 28be1591-3e89-4374-a31c-7e5cd1de6a04 · outbound

This paper cites New Horizons for Fundamental Physics with LISA.

Extreme mass ratio inspirals around topological stars New Horizons for Fundamental Physics with LISA

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.396047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.396047Z digest=sha256:f6118b62024b5317d5c096493235e0a6831cadd38bc00a5be7797d366f2b0627

Observation 3d39b34c-68fe-4dc5-8321-e8baf7acd181 · outbound

This paper cites Testing gravity with Extreme-Mass-Ratio Inspirals.

Extreme mass ratio inspirals around topological stars Testing gravity with Extreme-Mass-Ratio Inspirals

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.399609Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.399609Z digest=sha256:06be2702b974effda5de38da02129ce2e0be86956c3d91ee926ad5709928239a

Observation 51664ff0-86da-4300-a8cb-c563749c80a3 · outbound

This paper cites Can environmental effects spoil precision gravitational-wave astrophysics?.

Extreme mass ratio inspirals around topological stars Can environmental effects spoil precision gravitational-wave astrophysics?

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.403153Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.403153Z digest=sha256:b19a26d2a60e2876edf39047bc68689795f0fe95d10a5d9d46d4fa697231c24b

Observation 5d45c922-474c-4218-b360-4780b7e83e5d · outbound

This paper cites Probing the existence of ultralight bosons with a single gravitational-wave measurement.

Extreme mass ratio inspirals around topological stars Probing the existence of ultralight bosons with a single gravitational-wave measurement

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.407212Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.407212Z digest=sha256:5fdfb1a72524e53a52172b2461258fd7ed8e5c2f4b2cf49e21d8d4b1587dea35

Observation 71a352ec-77af-4569-8de2-adbf4cb22902 · outbound

This paper cites Probing time-dependent scalar wigs with extreme mass ratio inspirals.

Extreme mass ratio inspirals around topological stars Probing time-dependent scalar wigs with extreme mass ratio inspirals

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-08-16T11:17:28.974597Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-08-16T11:17:28.411126Z digest=sha256:372bfc03c81cec831d1d5a27463a5d47a76df9448e367de122ba20107a468ef4

Observation b99b5ec0-77b2-41f1-b0fa-1967c949b224 · outbound

This paper cites Gravitational waves from extreme-mass-ratio systems in astrophysical environments.

Extreme mass ratio inspirals around topological stars Gravitational waves from extreme-mass-ratio systems in astrophysical environments

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.415360Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.415360Z digest=sha256:8a972549a4d3d7a91c23e9ce1dcf56c048279299bfbfef1ac55d506dc79d7652

Observation 9daa4a32-3551-4737-973f-de1c9a47c501 · outbound

This paper cites Environmental effects in extreme mass ratio inspirals: perturbations to the environment in Kerr.

Extreme mass ratio inspirals around topological stars Environmental effects in extreme mass ratio inspirals: perturbations to the environment in Kerr

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.419739Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.419739Z digest=sha256:b2b7a3543c5fbdfde0f8f55f5e75230cbafef74028e74238cc6ca005b603deb1

Observation 5d445355-8d40-4a0b-8169-aa43f885f8ad · outbound

This paper cites Gravitational-wave signatures of the absence of an event horizon. II. Extreme mass ratio inspirals in the spacetime of a thin-shell gravastar.

Extreme mass ratio inspirals around topological stars Gravitational-wave signatures of the absence of an event horizon. II. Extreme mass ratio inspirals in the spacetime of a thin-shell gravastar

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.423882Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.423882Z digest=sha256:f3f024a132e45cabca34237313e188707c11e46b7293f8d85c9de0c96346cbb6

Observation fe941e51-46a9-4dd7-b451-c3dcae00c73d · outbound

This paper cites Distinguishing black holes from horizonless objects through the excitation of resonances during inspiral.

Extreme mass ratio inspirals around topological stars Distinguishing black holes from horizonless objects through the excitation of resonances during inspiral

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.427933Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.427933Z digest=sha256:6519c2358bef6186d8d1879734f304917b9b5896d02a2540487f03eeb0576af6

Observation 406340c0-4ed0-429f-af27-c92f0ef1945a · outbound

This paper cites Tidal heating as a discriminator for horizons in extreme mass ratio inspirals.

Extreme mass ratio inspirals around topological stars Tidal heating as a discriminator for horizons in extreme mass ratio inspirals

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.432257Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.432257Z digest=sha256:d12b8fc95d7699d107a3943bd2386d342c92115d3cbf6645a8fc91a7263ae0b1

Observation 3ba4acd7-f5be-4655-b552-94d233dee3aa · outbound

This paper cites Extreme mass-ratio inspirals around a spinning horizonless compact object.

Extreme mass ratio inspirals around topological stars Extreme mass-ratio inspirals around a spinning horizonless compact object

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.436345Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.436345Z digest=sha256:32a80f1a5192fa8593531248557c2d196fbb56eb91f562a9dbf0c581d365e30b

Observation 9787e0d8-ea8e-4182-a7bf-6a96f0dad9c1 · outbound

This paper cites Tidal heating as a discriminator for horizons in equatorial eccentric extreme mass ratio inspirals.

Extreme mass ratio inspirals around topological stars Tidal heating as a discriminator for horizons in equatorial eccentric extreme mass ratio inspirals

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.440496Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.440496Z digest=sha256:6f52d170a00ee7bf7f85243732d6b1aa8b25b4fa967b0059df9776a9bab8b880

Observation d7744df2-e0e6-4481-af4e-0713c89351a6 · outbound

This paper cites Gravitational Vacuum Condensate Stars.

Extreme mass ratio inspirals around topological stars Gravitational Vacuum Condensate Stars

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.444786Z

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source=pdf_text observed=2026-08-16T11:17:28.444786Z digest=sha256:00c1eacc3df69c515fc3e5527b36c715b3f7821961f6ea8ca3ad86c3575a3e04

Observation 9d0a4072-52d4-4061-bb19-d6837269bd74 · outbound

This paper cites Gravitational Condensate Stars: An Alternative to Black Holes.

Extreme mass ratio inspirals around topological stars Gravitational Condensate Stars: An Alternative to Black Holes

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.449019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.449019Z digest=sha256:d1dabb124a6910496c8ef36485080b676183e9756eca33d38a8cf28c7cb25db8

Observation bdba0ec1-abf2-4dbd-9269-5b138eab1df4 · outbound

This paper cites Topological Stars, Black holes and Generalized Charged Weyl Solutions.

Extreme mass ratio inspirals around topological stars Topological Stars, Black holes and Generalized Charged Weyl Solutions

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.453134Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.453134Z digest=sha256:43373433839bdd304ff4781ab23cc35e16ff2b89fb485d474b14771f3d253918

Observation da83d0c9-5cb5-4736-8ede-dfeacc40465e · outbound

This paper cites Bubble Bag End: A Bubbly Resolution of Curvature Singularity.

Extreme mass ratio inspirals around topological stars Bubble Bag End: A Bubbly Resolution of Curvature Singularity

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.457246Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.457246Z digest=sha256:6cca40a76545d3686a38367daf7eef46b2fcb1fae8c32bde24ccf08b62add256

Observation a1ae881e-41fe-40b3-ae82-b4c8515d5948 · outbound

This paper cites Probing Planckian corrections at the horizon scale with LISA binaries.

Extreme mass ratio inspirals around topological stars Probing Planckian corrections at the horizon scale with LISA binaries

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.461348Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.461348Z digest=sha256:4f6488c8565a4fa86e20191bcafd20df22d1f39efeebc007b82a1cb89b29f63b

Observation 7b43d3a6-9e53-495f-8555-ff7935b9ff40 · outbound

This paper cites Poisson, Phys.

Extreme mass ratio inspirals around topological stars Poisson, Phys

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.465484Z

Source-reported events for the cited work

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source=pdf_text observed=2026-08-16T11:17:28.465484Z digest=sha256:0494b630d953631a2b9c1464c80b7f4ef79fb59fc5deb28b41944ed0497ca8b6

Observation cbd3f962-92b9-4b91-964a-3150bfa7a84b · outbound

This paper cites Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections.

Extreme mass ratio inspirals around topological stars Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.469373Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.469373Z digest=sha256:bd5fde98b96b46a415669f6adb0a4b12bcbd1b75deee1c57ae7702d30a19a2a7

Observation d232fd0d-d963-4eed-a50e-2cb64de5b687 · outbound

This paper cites Calculable Corrections to Brane Black Hole Decay I: The Scalar Case.

Extreme mass ratio inspirals around topological stars Calculable Corrections to Brane Black Hole Decay I: The Scalar Case

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.473459Z

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source=pdf_text observed=2026-08-16T11:17:28.473459Z digest=sha256:71d6217a535164826797c6b09f06d86157fccdb98174732802dfe29b4c8402c0

Observation 0934ff46-3feb-4964-80fc-1633fb4f1a62 · outbound

This paper cites Greybody Factors for Rotating Black Holes on Codimension-2 Branes.

Extreme mass ratio inspirals around topological stars Greybody Factors for Rotating Black Holes on Codimension-2 Branes

Reference 70

Resolution
verified exact
local_arxiv, observed 2026-08-16T11:17:28.772560Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-08-16T11:17:28.477551Z digest=sha256:c397cd8cdcd91738ebcf31721844433e1038d511c1800573b3df008ff561db39

Observation 031ee6ef-3701-42bc-b6a7-4733c98f5e8b · outbound

This paper cites Scalar Emission in the Bulk in a Rotating Black Hole Background.

Extreme mass ratio inspirals around topological stars Scalar Emission in the Bulk in a Rotating Black Hole Background

Reference 71

Resolution
verified exact
local_arxiv, observed 2026-08-16T11:17:28.754408Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-08-16T11:17:28.481346Z digest=sha256:e310e5b1ff66c4da2f2e7043f6dde8793e63e892a1e89fa2f0b80b629f7bd27c

Observation eedcd763-d595-4ef3-ab75-55cf2a635a07 · outbound

This paper cites Tidal effects around higher-dimensional black holes.

Extreme mass ratio inspirals around topological stars Tidal effects around higher-dimensional black holes

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.484870Z

Source-reported events for the cited work

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source=pdf_text observed=2026-08-16T11:17:28.484870Z digest=sha256:c269948d267ae3533bab42b9bac7b529c49c7b6bb12a87f7eb5a03a9668abafc

Observation a939d1e0-5a4e-413d-a148-fa7e7cae5e4f · outbound

This paper cites an unresolved cited work.

Extreme mass ratio inspirals around topological stars Unresolved cited work

Reference 73

Resolution
unresolved
raw_fallback, observed 2026-08-16T11:17:29.738084Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-08-16T11:17:28.488592Z digest=sha256:64dfa6302f50982e1f049c3d08f28907480e683c70d69e1cf8b909025e5a228f

Observation f30c8a51-d7cb-4ba9-a8aa-2e9b79cf039c · outbound

This paper cites Light rings as observational evidence for event horizons: long-lived modes, ergoregions and nonlinear instabilities of ultracompact objects.

Extreme mass ratio inspirals around topological stars Light rings as observational evidence for event horizons: long-lived modes, ergoregions and nonlinear instabilities of ultracompact objects

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.491906Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.491906Z digest=sha256:db60a678e700aa373e9db1c806cb0697851cf2cbdede09b8fa40ed902b6d38c5

Observation 26302060-99b9-4db7-a9cc-ede497087231 · outbound

This paper cites an unresolved cited work.

Extreme mass ratio inspirals around topological stars Unresolved cited work

Reference 75

Resolution
verified exact
raw_fallback, observed 2026-08-16T11:17:28.708074Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-08-16T11:17:28.495979Z digest=sha256:7de27b9f172d38ce4016bd215d6df8bce30cf329c579bfadc86d82ca14b982dc

Observation 34ce57cd-eebf-41c5-98ac-feeea12348ce · outbound

This paper cites Model Waveform Accuracy Standards for Gravitational Wave Data Analysis.

Extreme mass ratio inspirals around topological stars Model Waveform Accuracy Standards for Gravitational Wave Data Analysis

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.499848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.499848Z digest=sha256:56fe7fb2191b0a29a217bf1e0bad6b9f7de785b1b3796c1ae45e994039309b16

Observation ea8a129b-19b7-4287-a7b4-5f112c84f06b · outbound

This paper cites Microstates of Non-extremal Black Holes: A New Hope.

Extreme mass ratio inspirals around topological stars Microstates of Non-extremal Black Holes: A New Hope

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.503976Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.503976Z digest=sha256:2c2a042ee2413b41b1d50d4da53bd5687b6b15f36d15ce79bb288e4be57bf07d

Observation 54405976-691c-41d4-a001-b712620d3df6 · outbound

This paper cites Rotating Topological Stars.

Extreme mass ratio inspirals around topological stars Rotating Topological Stars

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.508089Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:17:28.508089Z digest=sha256:6af3d36ec8d7fbc6a736a56efbb33a5bcf5ae4563799d1efdbac0e473142b2f3

Observation 4ef701e8-c91a-405d-a633-de1c62edacc1 · outbound

This paper cites an unresolved cited work.

Extreme mass ratio inspirals around topological stars Unresolved cited work

Reference 79

Resolution
unresolved
raw_fallback, observed 2026-08-16T11:17:29.724473Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

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Observation 4e6411ee-8150-456a-9691-e476710b55d3 · outbound

This paper cites Waveform Modelling for the Laser Interferometer Space Antenna.

Extreme mass ratio inspirals around topological stars Waveform Modelling for the Laser Interferometer Space Antenna

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.516467Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 5c986b57-377f-4fea-a8fb-85798c5daf41 · outbound

This paper cites Advanced Methods in Black-Hole Perturbation Theory.

Extreme mass ratio inspirals around topological stars Advanced Methods in Black-Hole Perturbation Theory

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.520583Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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This paper cites Perturbations of slowly rotating black holes: massive vector fields in the Kerr metric.

Extreme mass ratio inspirals around topological stars Perturbations of slowly rotating black holes: massive vector fields in the Kerr metric

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-16T11:17:28.524800Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Pith citing papers

Observation ac2901c9-d4ad-4e31-8b5b-dd62ebdd6d35 · inbound

Topological Stars and scalar wave equation: Exact resummation of the renormalized angular momentum in the eikonal limit cites this paper.

Topological Stars and scalar wave equation: Exact resummation of the renormalized angular momentum in the eikonal limit Extreme mass ratio inspirals around topological stars

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-07T00:32:36.527524Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 7c633c70-745b-4e52-8ec1-dae429e30ffd · inbound

Gravitational Atoms from Topological Stars cites this paper.

Gravitational Atoms from Topological Stars Extreme mass ratio inspirals around topological stars

Reference 50

Resolution
verified exact
arxiv_id, observed 2026-05-17T22:50:25.882904Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

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Observation 957bb4bf-9e11-4b92-889d-ceaee0c4d321 · inbound

Taxonomy of periodic orbits and gravitational waves in a non-rotating Destounis-Suvorov-Kokkotas black hole spacetime cites this paper.

Taxonomy of periodic orbits and gravitational waves in a non-rotating Destounis-Suvorov-Kokkotas black hole spacetime Extreme mass ratio inspirals around topological stars

Reference 38

Resolution
verified exact
arxiv_id, observed 2026-05-16T18:41:11.039670Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

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